A High-Temperature Al–Ca Condensate in the Lunar Regolith
- Authors: Mokhov A.V.1, Gornostaeva T.A.1, Kartashov P.M.1, Rybchuk A.P.1, Bogatikov O.A.1
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Affiliations:
- Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)
- Issue: Vol 487, No 1 (2019)
- Pages: 815-818
- Section: Geochemistry
- URL: https://journals.rcsi.science/1028-334X/article/view/195250
- DOI: https://doi.org/10.1134/S1028334X1907016X
- ID: 195250
Cite item
Abstract
For the first time, a high-temperature condensate in the form of two-component glass beads of about 200–400 nm size, consisting of an Al–Ca oxide core rimmed by a uniform oxide film of high-silica glass containing iron nano-inclusions, has been found in natural samples of the lunar regolith from Mare Crisium (Luna-24). Earlier, a high-temperature condensate was only theoretically predicted on the basis of laser evaporation experiments.
About the authors
A. V. Mokhov
Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)
Author for correspondence.
Email: avm8okhov@gmail.com
Russian Federation, Moscow, 119017
T. A. Gornostaeva
Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)
Email: avm8okhov@gmail.com
Russian Federation, Moscow, 119017
P. M. Kartashov
Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)
Email: avm8okhov@gmail.com
Russian Federation, Moscow, 119017
A. P. Rybchuk
Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)
Email: avm8okhov@gmail.com
Russian Federation, Moscow, 119017
O. A. Bogatikov
Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)
Email: avm8okhov@gmail.com
Russian Federation, Moscow, 119017